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Table 2
Literature values compared to our adopted effective temperature, surface gravity, and metallicity.
HD 209458 | ||||
Teff [K] | log g [cm s-2] | [Fe/H] | Reference | Method |
|
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6000 | 4.25 | 0.00 | Mazeh et al. (2000) | spectroscopic |
6063 | 4.38 | 0.04 | Gonzalez et al. (2001) | spectroscopic |
6080 | 4.33 | −0.06 | Mashonkina & Gehren (2001) | spectroscopic |
5987 | 4.24 | −0.04 | Sadakane et al. (2002) | spectroscopic |
6100 | 4.50 | −0.02 | Heiter & Luck (2003) | spectroscopic |
6117 | 4.48 | 0.02 | Santos et al. (2004) | spectroscopic |
5993 | Ramírez & Meléndez (2004) | photometric | ||
6099 | 4.38 | 0.02 | Valenti & Fischer (2005) | spectroscopic |
6118 | 4.50 | 0.03 | Sousa et al. (2008) | spectroscopic |
4.368 | Southworth (2009) | light curve | ||
6108 | 4.33 | −0.04 | Casagrande et al. (2011) | photometric |
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6095 | 4.3 | 0.00 | adopted (3D model) | spectroscopic |
6000 | 4.3 | 0.00 | adopted (1D model) | spectroscopic |
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HD 189733 | ||||
Teff [K] | log g [cm s-2] | [Fe/H] | Reference | Method |
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5050 | 4.53 | −0.03 | Bouchy et al. (2005) | spectroscopic |
4939 | van Belle & von Braun (2009) | photometric | ||
4.610 | Southworth (2010) | light curve | ||
5022 | 4.58 | −0.13 | Casagrande et al. (2011) | photometric |
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5050 | 4.53 | 0.00 | adopted (3D model) | spectroscopic |
5000 | 4.53 | 0.00 | adopted (1D model) | spectroscopic |
Notes. Quoted metallicities could not be corrected for differences in the assumed solar composition, as the latter was not always specified in the cited publications, leading to artificial offsets in [Fe/H].
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